Zobrazeno 1 - 10
of 1 012
pro vyhledávání: '"Parrent A"'
Autor:
Arévalo-Astrada, Miguel A., Suller-Marti, Ana, McLachlan, Richard S., Paredes-Aragón, Elma, Jones, Michelle-Lee, Parrent, Andrew G., Mirsattari, Seyed M., Lau, Jonathan C., Steven, David A., Burneo, Jorge G.
Publikováno v:
In Epilepsy Research December 2023 198
An examination of late-time, optical spectra of type Ia supernovae revealed surprisingly narrow absorption features which only become visible a few months after maximum light. These features, most clearly seen in the late-time spectra of the bright,
Externí odkaz:
http://arxiv.org/abs/1810.06788
Autor:
Coppejans, D. L., Margutti, R., Guidorzi, C., Chomiuk, L., Alexander, K. D., Berger, E., Bietenholz, M. F., Blanchard, P. K., Challis, P., Chornock, R., Drout, M., Fong, W., Mac Fadyen, A., Migliori, G., Milisavljevic, D., Nicholl, M., Parrent, J. T., Terreran, G., Zauderer, B. A.
The energy source powering the extreme optical luminosity of hydrogen-stripped Superluminous Supernovae (SLSNe-I) is not known, but recent studies have highlighted the case for a central engine. Radio and/or X-ray observations are best placed to trac
Externí odkaz:
http://arxiv.org/abs/1711.03428
Autor:
Graham, Melissa L., Kumar, Sahana, Hosseinzadeh, Griffin, Hiramatsu, Daichi, Arcavi, Iair, Howell, D. Andrew, Valenti, Stefano, Sand, David J., Parrent, Jerod T., McCully, Curtis, Filippenko, Alexei V.
We present late-time spectra of eight Type Ia supernovae (SNe Ia) obtained at $>200$ days after peak brightness using the Gemini South and Keck telescopes. All of the SNe Ia in our sample were nearby, well separated from their host galaxy's light, an
Externí odkaz:
http://arxiv.org/abs/1708.07799
Autor:
Law, Charles J., Milisavljevic, Dan, Crabtree, Kyle N., Johansen, Sommer L., Patnaude, Daniel J., Margutti, Raffaella, Parrent, Jerod T., Drout, Maria R., Sanders, Nathan E., Kirshner, Robert P., Latham, David W.
Diffuse interstellar bands (DIBs) are absorption features commonly observed in optical/near-infrared spectra of stars and thought to be associated with polyatomic molecules that comprise a significant reservoir of organic material in the universe. Ho
Externí odkaz:
http://arxiv.org/abs/1706.07801
Autor:
Milisavljevic, D., Patnaude, D., Raymond, J., Drout, M., Margutti, R., Kamble, A., Chornock, R., Guillochon, J., Sanders, N., Parrent, J., Lovisari, L., Chilingarian, I., Challis, P., Kirshner, R., Penny, M., Itagaki, K., Eldridge, J. J., Moriya, T.
The progenitor systems of the class of "Ca-rich transients" is a key open issue in time domain astrophysics. These intriguing objects exhibit unusually strong calcium line emissions months after explosion, fall within an intermediate luminosity range
Externí odkaz:
http://arxiv.org/abs/1706.01887
Autor:
Shivvers, Isaac, Zheng, WeiKang, Van Dyk, Schuyler D., Mauerhan, Jon, Filippenko, Alexei V., Smith, Nathan, Foley, Ryan J., Mazzali, Paolo, Kamble, Atish, Kilpatrick, Charles D., Margutti, Raffaella, Yuk, Heechan, Graham, Melissa L., Kelly, Patrick L., Andrews, Jennifer, Matheson, Thomas, Wood-Vasey, W. M., Ponder, Kara A., Brown, Peter J., Chevalier, Roger, Milisavljevic, Dan, Drout, Maria, Parrent, Jerod, Soderberg, Alicia, Ashall, Chris, Piascik, Andrzej, Prentice, Simon
Publikováno v:
2017MNRAS.471.4381S
We present the results of an extensive observational campaign on the nearby Type Ibn SN 2015G, including data from radio through ultraviolet wavelengths. SN 2015G was asymmetric, showing late-time nebular lines redshifted by ~1000 km/s. It shared man
Externí odkaz:
http://arxiv.org/abs/1704.04316
Autor:
Suller Marti, Ana, Mirsattari, Seyed M., Steven, David A., McLachlan, Richard S., Parrent, Andrew G., Hayman-Abello, Susan, MacDougall, Keith W., Andrade, Andrea, de Ribaupierre, Sandrine, Diosy, David C., Burneo, Jorge G.
Publikováno v:
In Clinical Neurology and Neurosurgery March 2022 214
Autor:
Lunnan, R., Kasliwal, M. M., Cao, Y., Hangard, L., Yaron, O., Parrent, J. T., McCully, C., Gal-Yam, A., Mulchaey, J. S., Ben-Ami, S., Filippenko, A. V., Fremling, C., Fruchter, A. S., Howell, D. A., Koda, J., Kupfer, T., Kulkarni, S. R., Laher, R., Masci, F., Nugent, P. E., Ofek, E. O., Yagi, M., Yan, Lin
Publikováno v:
The Astrophysical Journal (2017), 836, 60
We present the Palomar Transient Factory discoveries and the photometric and spectroscopic observations of PTF11kmb and PTF12bho. We show that both transients have properties consistent with the class of calcium-rich gap transients, specifically lowe
Externí odkaz:
http://arxiv.org/abs/1612.00454
Autor:
Friesen, Brian, Baron, E., Parrent, Jerod T., Thomas, R. C., Branch, David, Nugent, Peter, Hauschildt, Peter H., Foley, Ryan J., Wright, Darryl E., Pan, Yen-Chen, Filippenko, Alexei V., Clubb, Kelsey I., Silverman, Jeffrey M., Maeda, Keiichi, Shivvers, Isaac, Kelly, Patrick L., Cohen, Daniel P., Rest, Armin, Kasen, Daniel
We present optical spectra of the nearby Type Ia supernova SN 2011fe at 100, 205, 311, 349, and 578 days post-maximum light, as well as an ultraviolet spectrum obtained with Hubble Space Telescope at 360 days post-maximum light. We compare these obse
Externí odkaz:
http://arxiv.org/abs/1607.04784